<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Andronov, I. L.</style></author><author><style face="normal" font="default" size="100%">Baklanov, A. V.</style></author><author><style face="normal" font="default" size="100%">Chinarova, L. L.</style></author><author><style face="normal" font="default" size="100%">Chochol, D.</style></author><author><style face="normal" font="default" size="100%">Gazeas, K.</style></author><author><style face="normal" font="default" size="100%">Halevin, A. V.</style></author><author><style face="normal" font="default" size="100%">Kolesnikov, S. V.</style></author><author><style face="normal" font="default" size="100%">Kudashkina, L. S.</style></author><author><style face="normal" font="default" size="100%">Marsakova, V. I.</style></author><author><style face="normal" font="default" size="100%">Mason, P. A.</style></author><author><style face="normal" font="default" size="100%">Niarchos, P. G.</style></author><author><style face="normal" font="default" size="100%">Patkos, L.</style></author><author><style face="normal" font="default" size="100%">Pavlenko, E. P.</style></author><author><style face="normal" font="default" size="100%">Shakhovskoy, N. M.</style></author><author><style face="normal" font="default" size="100%">Shapovalova, L. L.</style></author><author><style face="normal" font="default" size="100%">Tremko, J.</style></author><author><style face="normal" font="default" size="100%">Zola, S.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Periodic and aperiodic variability of the interacting binary and long-periodic stars</style></title><short-title><style face="normal" font="default" size="100%">Kinematika i Fizika Nebesnykh Tel Supplement</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2000</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2000/09/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2000KFNTS...3..383A</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">3</style></volume><pages><style face="normal" font="default" size="100%">383 - 388</style></pages><isbn><style face="normal" font="default" size="100%">0233-7665</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">Recent results obtained within the framework of the international observational and research campaigns are reviewed. The main topics are following: magnetic cataclysmic variables: synchronization of the spin and orbital period of the white dwarf; observational evidence on the switching of the accretion from one pole to another; non-dipole configuration of the magnetic field; ``swingings'' of the orientation of the magnetic axis in the `` synchronous systems''; instability of the accretion and the ``red noise''; long-term luminosity changes; UV Cet - like flares; two-pole accretion in the intermediate polars; weakly- and non- magnetic cataclysmic variables: negative and positive superhumps in the nova-like variables; ``red noise'' and/or quasi-periodic oscillations; unprecedented switch of the superhump period in TT Ari; the luminosity dependence of the superhump period in BZ Cam and V725 Aql; long-term variations of the outburst characteristics of dwarf novae and luminosity of old novae - magnetic activity of the red secondary vs third body orbiting around a cataclysmic variable; symbiotic binaries: light curve variations in symbiotic novae and stars with a pulsating component; long-periodic pulsating variables: statistical study of the characteristics of the mean phase curves and of the individual cycles; additional classification criteria for the Mira-type and semi-regular stars. Some of the original papers are available at http://www.paco.odessa.ua/~il-a and http://ila.webjump.com</style></abstract></record></records></xml>